Two articles published in the journal “Monthly Notices of the Royal Astronomical Society: Letters” report different aspects of a study on two anomalous stars, as they’re two subdwarfs that have carbon and oxygen on the surface instead of hydrogen and helium. A team led by Professor Klaus Werner of the German University of Tübingen discovered the two stars, cataloged as PG 1654+322 and PG 1528+025 as part of a research aimed at better understanding the final stages of stellar evolution. A team led by Dr. Miller Bertolam of the Institute of Astrophysics of La Plata, Argentina, offered a possible explanation for the two anomalous stars by explaining in one of two articles that they could have formed as a result of mergers between two white dwarfs.